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Article

Existence of Bounded Solutions for a Class of Degenerate Fourth-Order Elliptic Equations with Convection Terms

by
Salvatore D’Asero
Dipartimento di Matematica e Informatica, University of Catania, Viale A. Doria 6, 95125 Catania, Italy
Mathematics 2025, 13(1), 3; https://doi.org/10.3390/math13010003
Submission received: 11 November 2024 / Revised: 11 December 2024 / Accepted: 18 December 2024 / Published: 24 December 2024
(This article belongs to the Special Issue Problems and Methods in Nonlinear Analysis)

Abstract

:
This paper deals with the existence of bounded and locally Hölder continuous weak solutions of the following nonlinear fourth-order Dirichlet problem: | α | = 1 , 2 ( 1 ) | α | D α A α ( x , u , D 1 u , D 2 u ) E α ( x )   | u | λ ( p α 1 )   sign u = f in Ω , where the coefficients A α satisfy a strengthened degenerate coercivity condition.

1. Introduction

In the present article, we consider the following nonlinear fourth-order equation with convection terms:
| α | = 1 , 2 ( 1 ) | α | D α A α ( x , u , D 1 u , D 2 u ) E α ( x )   | u | λ ( p α 1 )   sign u = f   in   Ω
where Ω R N , N 3 , is an open bounded set, α = ( α 1 , , α N ) is a multi-index with non-negative integer components and length | α | = α 1 + + α N , and D α u ( x ) = | α | u ( x ) x 1 α 1 x 2 α 2 x N α N , D h u = D α u : | α | = h , for h = 1 , 2 .
The coefficients A α satisfy the following coercivity condition:
| α | = 1 , 2 A α ( x , η , ξ ) ξ α ν 1 | α | = 1 , 2 | ξ α | p α ( 1 + | η | ) θ ( p α 1 ) ,
where θ , λ and p α are real numbers such that 0 θ < 1 , 0 < λ < 1 and
p α = q if   | α | = 1 p if   | α | = 2
with 1 < p < N 2 , 2 p < q < N . The terms E α , | α | = 1 , 2 , and f are a vector field and a function, respectively, satisfying suitable summability assumptions.
The coercivity condition (2) was introduced by I. V. Skrypnik in 1978 in [1] for the case θ = 0 in the framework of higher-order equations (with E α 0 , | α | = 1 , 2 ) in order to prove the boundedness and Holder continuity of the solutions. It turns out that this condition is stronger than the one usually considered for nonlinear fourth-order elliptic equations, i.e.,
| α | = 2 A α ( x , ξ ) ξ α ν 1 | α | = 2 | ξ α | p ν 2 | α | < 2 | ξ α | s α f ( x ) ,
which, unfortunately, does not even ensure the boundedness of the solutions (see well-known counterexamples in [2,3,4]) unless 2 p > N (as a consequence of Sobolev’s embedding theorem) or 2 p = N (see [5]) or N 2 p is sufficiently small (see [6]).
Operators satisfying condition (2) with θ = 0 have been studied in connection with many other questions, such as L 1 -theory, the qualitative properties of the solutions, and removable singularities in the degenerate and non-degenerate cases in [7,8,9,10,11,12]. Moreover, existence and regularity results for the solutions of a class of nonlinear fourth-order equations, with the principal part satisfying (2) with θ = 0 and lower-order terms having so-called “natural growth”, were obtained in [13,14,15,16,17].
In dealing with the boundary-value problem related to Equation (1), two difficulties arise. Firstly, the nonlinear fourth-order operator
u | α | = 1 , 2   ( 1 ) | α | D α A α ( x , u , D 1 u , D 2 u )
under condition (2), though well defined, is not coercive on W 0 1 , q ( Ω ) W 0 2 , p ( Ω ) when u is large. Moreover, due to the presence of the convection term, the operator
u | α | = 1 , 2 ( 1 ) | α | D α A α ( x , u , D 1 u , D 2 u ) E α   | u | λ ( p α 1 ) sign ( u )
may be not be coercive even if θ = 0 , unless we assume that the sizes of the norm | | E α | | L N | α | ( p α 1 ) ( Ω ) , | α | = 1 , 2 , are sufficiently small, or | α | = 1 , 2 D α E α = 0 .
To overcome the lack of coercivity, we approximate our problem with a sequence of homogeneous non-degenerate Dirichlet problems, and we prove an L a priori estimate on the approximating solutions, which, in turn, implies an a priori estimate in the energy space. Once this has been accomplished, a compactness result for the approximating solutions allows us to find a bounded weak solution of the boundary-value problem related to Equation (1), which is also locally Hölder continuous.
In the framework of the second-order Dirichlet problem, the model problem
div u ( 1 + | u | ) θ E ( x )   | u | λ sign u = f   in   Ω in   Ω u = 0 on   Ω
was studied in [18], where the authors obtained existence and regularity results under various assumptions on f (see [19,20] in the case E 0 ).
It is well known that when dealing with fourth-order equations, some difficulties arise. As a matter of fact, the corresponding weak formulation contains terms related to second-order derivatives of test functions that must be correctly taken into account.
This article is organized as follows. In Section 2, we formulate the hypotheses and state the results. In Section 3, we present some auxiliary lemmas, and we prove a priori estimates that will be used in the proof of the boundedness theorem. In Section 4, we provide proof of the existence of a bounded solution. Finally, the Hölder continuity of bounded solutions is proved in Section 5.

2. Preliminaries and Statement of Results

Let Ω be an open bounded set in R N with N 3 . We denote by N ( 2 ) the number of different multi-indices α such that | α | = 1 , 2 .
Let A α ( x , η , ξ ) : Ω × R × R N ( 2 ) R , with | α | = 1 , 2 , be Carathéodory functions (i.e., A α ( · , η , ξ ) is measurable on Ω for every ( η , ξ ) R × R N ( 2 ) , and A α ( x , · , · ) is continuous on R × R N ( 2 ) for almost every x Ω ), satisfying the following structural conditions for almost every x Ω , every η R and ξ , ξ R N ( 2 ) , ξ ξ :
| α | = 1 , 2 A α ( x , η , ξ ) ξ α ν 1 | α | = 1 , 2 | ξ α | p α ( 1 + | η | ) θ ( p α 1 ) ,
| α | = 1 , 2 | A α ( x , η , ξ ) | p α p α 1 ν 2 | α | = 1 | ξ α | q + | α | = 2 | ξ α | p ,
| α | = 1 , 2 A α ( x , η , ξ ) A α ( x , η , ξ ) ( ξ α ξ α ) > 0 ,
where ν 1 , ν 2 are positive constants, 0 θ < 1 , and p α , | α | = 1 , 2 , is defined by (3). Let E α ( x )   :   Ω R N , | α | = 1 , and E α ( x )   :   Ω R N 2 , | α | = 2 , be vector fields such that
| E α | L r α ( Ω )   with   r α > N | α | ( p α 1 ) ,   | α | = 1 , 2
and
f L t ( Ω )   with   t > N / q .
We set
W 2 , p 1 , q ( Ω ) = W 1 , q ( Ω ) W 2 , p ( Ω ) ,
and
W ˚ 2 , p 1 , q ( Ω ) = W 0 1 , q ( Ω ) W 0 2 , p ( Ω ) .
Assumptions (5)–(9) allow us to give the following definition.
Definition 1. 
A weak solution of the problem
| α | = 1 , 2 ( 1 ) | α | D α A α ( x , u , D 1 u , D 2 u ) E α   | u | λ ( p α 1 ) sign u = f in   Ω D α u = 0 ,   | α | = 0 , 1 on   Ω
is a function u W ˚ 2 , p 1 , q ( Ω ) such that the integral identity
| α | = 1 , 2   Ω A α ( x , u , D 1 u , D 2 u ) D α v   d x = | α | = 1 , 2   Ω E α | u | λ ( p α 1 ) 1   u   D α v   d x     + Ω f v   d x
holds for every v W ˚ 2 , p 1 , q ( Ω ) .
Our first result states the existence of a bounded weak solution of (10).
Theorem 1. 
Let us suppose that conditions (5)–(9) are satisfied, and
0 θ < q p p ( q 1 )   and   θ + λ < 1 .
Then, there exists a weak solution u of problem (10), in the sense of Definition 1, such that
u L ( Ω ) M
where M > 0 is a constant depending on θ , N, q, p, ν 1 , ν 2 , | Ω | , E α L r α ( Ω ) , | α | = 1 , 2 and | | f | | L t ( Ω ) .
Furthermore, under the same assumptions as Theorem 1, the local Hölder continuity of any weak solution u W ˚ 2 , p 1 , q ( Ω ) L ( Ω ) holds, as stated in the following theorem.
Theorem 2. 
Let us suppose that conditions (5)–(9) and (12) are satisfied. Let u W ˚ 2 , p 1 , q ( Ω ) be a bounded solution of problem (10). Then, there exists ρ ( 0 , 1 ) , depending on θ , N, q, p, ν 1 , ν 2 , | Ω | , E α L r α ( Ω ) , | α | = 1 , 2 , and | | f | | L t ( Ω ) and on | | u | | L ( Ω ) , such that u C l o c 0 , ρ ( Ω ) , and, for any domain Ω Ω , we have
| u ( x ) u ( y ) | C | x y | ρ   for   any   x , y Ω
where C is a positive constant depending on the same parameters as ρ, and d = dist ( Ω , Ω ) .
Remark 1. 
Assumption (9) on f, required in Theorems 1 and 2, is the same one that yields the existence of bounded and Hölder continuous solutions for fourth-order equations satisfying the degenerate condition (5) and E α 0 , | α | = 1 , 2 (see [21]), as well as for non-degenerate (i.e., θ = 0 ) fourth-order equations and E α 0 , | α | = 1 , 2 (see [22]). In the latter case, examples of unbounded solutions of Equation (1) with f L N q ( Ω ) and f L N q + ε ( Ω ) , for every ε > 0 , are constructed in [23]. On the other hand, hypothesis (9) is also required to prove the boundedness and Hölder continuity of the solutions of Equation (1), where λ = 1 and the coefficients A α ( x , η , ξ ) satisfy condition (5) with θ = 0 (see [24]).

3. Auxiliary Lemmas and a Priori Estimates

We begin this section by recalling an algebraic lemma according to Serrin (see Lemma 2 in [25]).
Lemma 2. 
Let χ be a positive exponent and a i , β i , i = 1 , , m , be two sets of m real numbers such that 0 < a i < + and 0 < β i < χ . Suppose that z is a positive number satisfying the inequality
z χ i = 1 m a i z β i .
Then,
z C i = 1 m a i γ i ,
where C depends only on m, χ, β i and γ i = 1 χ β i , i = 1 , , m .
Moreover, we present a slightly modified version of Stampacchia’s well-known lemma (see [26]), whose proof is contained in [19,22]. See also [27] for new generalizations.
Lemma 3. 
Let ϕ :   R + R + be a non-increasing function such that
ϕ ( h ) c 0 ( h k ) ν k τ ν [ ϕ ( k ) ] 1 + μ ,   for   all   h > k k 0 > 0 ,
for some positive constants c 0 and k 0 , with ν > 0 , 0 τ < 1 and μ > 0 . Then, there exists k * > 0 , depending on c 0 , τ, ν, μ and k 0 , such that ϕ ( k * ) = 0 .
Finally, we recall the following lemma, which ensures that the composition of a C 2 function ζ ( s ) with a function u W ˚ 2 , p 1 , q ( Ω ) belongs to W ˚ 2 , p 1 , q ( Ω ) .
Lemma 4 
([28] Proposition 9.5). Let ζ C 2 ( R ) be a function with bounded derivatives ζ and ζ such that ζ ( 0 ) = 0 . If u W ˚ 2 , p 1 , q ( Ω ) , then
ζ ( u ) W ˚ 2 , p 1 , q ( Ω ) ,
and for each multi-index α such that | α | = 1 , 2 , the following assertion holds:
D α ζ ( u ) = ζ ( u ) D α u + R | α | ( u )
where, for i.e., x Ω ,
R | α | ( u ) = 0 i f   | α | = 1 ζ ( u ) | β | = | γ | = 1 D β u D γ u i f   | α | = 2 .  
Given n N , let T n ( s ) be the truncation function defined by
T n ( s ) = s if   | s | n n   sign ( s ) if   | s | > n .
Following the technique already used in [19,20] in the framework of second-order elliptic equations, let us define the following Dirichlet problems:
u n W ˚ 2 , p 1 , q ( Ω ) , | α | = 1 , 2   Ω A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) D α v   d x   = | α | = 1 , 2   Ω E α u n 1 n + | u n |   | u n | λ ( p α 1 ) 1 + 1 n | u n | λ ( p α 1 ) D α v   d x + Ω f v   d x for   every   v W ˚ 2 , p 1 , q ( Ω ) .
By Schauder’s fixed-point theorem, there exists a solution u n W ˚ 2 , p 1 , q ( Ω ) of problem (15). Moreover, since, for every fixed n N ,
u n 1 n + | u n |   | u n | λ ( p α 1 ) 1 + 1 n | u n | λ ( p α 1 ) n   for   i . e . ,   x Ω
under conditions (8) and (9), every u n is bounded thanks to the boundedness result of [22] (see also [14]).
The next two lemmas are crucial for passing to the limit in the approximating problems (15). The first one concerns the equi-boundedness of the sequence u n .
Lemma 5. 
Assume that conditions (5)–(9) and (12) are satisfied. Let u n be a solution of problem (15) for every n N . Then, there exists a positive constant M, depending only on θ , λ, N, q, p, ν 1 , ν 2 , | Ω | , E α L r α ( Ω ) , | α | = 1 , 2 and | | f | | L t ( Ω ) , such that
| | u n | | L ( Ω ) M   for   every   n N .
Proof. 
Given k 1 and σ > 2 , let us consider the function
ζ ( s ) = | s | θ ( q 1 )   | s | k + σ sign ( s ) .
Due to the boundedness of u n and thanks to Lemma 4, ζ ( u n ) is an admissible test function in (15). Moreover,
D α ζ ( u n ) = σ + θ ( q 1 ) | u n | k + | u n |   | u n | θ ( q 1 )   | u n | k + σ 1 D α u n + R | α | ( u n )
where, for i.e., x Ω ,
R | α | ( u n ) = 0 if   | α | = 1 | R | α | ( u n ) | σ 2 θ 2 q 2   | u n | θ ( q 1 )   | u n | k + σ 2 | β | = 1 | D β u n | 2 if   | α | = 2 .
Note that we have used the inequality
0 | u n | k + | u n | 1 ,   for   any   k 0 .
We test the integral identity (15) with v = ζ ( u n ) . Using condition (5) and inequality (19), we obtain
ν 1 σ | α | = 1 , 2 Ω | D α u n | p α   | u n | θ ( q 1 ) ( 1 + | T n ( u n ) | ) θ ( p α 1 ) | u n | k + σ 1   d x   | α | = 1 , 2 Ω A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) [ σ   | u n | θ ( q 1 ) | u n | k + σ 1 + θ ( q 1 ) | u n | θ ( q 1 ) 1   | u n | k + σ ] D α u n   d x   c { | α | = 2 Ω | A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) | | R | α | ( u n ) |   d x   + | α | = 1 , 2 Ω | E α |   | u n | λ ( p α 1 ) + θ ( q 1 )   | u n | k + σ 1 | D α u n |   d x + | α | = 2 Ω | E α |   | u n | λ ( p α 1 ) | R | α | ( u n ) |   d x + Ω | f |   | u n | θ ( q 1 ) | u n | k + σ   d x }   = c I 1 + J α + I 2 + Ω | f |   | u n | θ ( q 1 ) | u n | k + σ   d x .
From now on, we denote by c a positive constant that does not depend on n (namely, it may depend on N, | Ω | , θ , λ , σ , p, q, ν 1 , ν 2 and E α L r α ( Ω ) f L t ( Ω ) ) and whose value may vary from line to line.
Let us evaluate the integrals on the right-hand side of (20).
We observe that the following inequality holds:
1 + | T n ( u n ) | 1 + | u n | ,   for   any   n N .
Using Young’s inequality with the exponents p α and p α p α 1 , for all τ > 0 , we obtain
J α τ | α | = 1 , 2 Ω | D α u n | p α   | u n | θ ( q 1 ) ( 1 + | T n ( u n ) | ) θ ( p α 1 ) | u n | k + σ 1   d x           + C ( c , τ ) | α | = 1 , 2 Ω | E α | p α p α 1   1 + | u n | λ p α + q θ | u n | k + σ 1   d x .  
The growth condition (6), estimate (18) and, again, Young’s inequality with the exponents p p 1 , q 2 and δ = p q q 2 p give us, for all τ > 0 and σ > 1 + δ ,
I 1 c Ω | α | = 1 , 2 | D α u n | p α p 1 p | u n | θ ( q 1 )   | u n | k + σ 2 | α | = 1 | D α u n | 2   d x   τ | α | = 1 , 2 Ω | D α u n | p α   | u n | θ ( q 1 ) ( 1 + | T n ( u n ) | ) θ ( p α 1 ) | u n | k + σ 1   d x       + C ( c , τ ) Ω 1 + | u n | θ ( q 1 ) δ | u n | k + σ 1 δ   d x .  
and
I 2 c | α | = 2 Ω | E α |   | u n | λ ( p 1 ) + θ ( q 1 ) | u n | k + σ 2 | α | = 1 | D α u n | 2   d x       τ | α | = 1 Ω | D α u n | q   | u n | θ ( q 1 ) ( 1 + | T n ( u n ) | ) θ ( q 1 ) | u n | k + σ 1   d x       + C ( c , τ ) [ | α | = 2 Ω | E α | p p 1   1 + | u n | λ p + q θ | u n | k + σ 1   d x   + Ω 1 + | u n | θ ( q + δ ) | u n | k + σ 1 δ   d x ] .  
From (20), thanks to (22)–(24) and choosing a suitable 0 < τ < 1 , we deduce
Ω | α | = 1 , 2 | D α u n | p α   | u n | θ ( q 1 ) ( 1 + | T n ( u n ) | ) θ ( p α 1 ) | u n | k + σ 1   d x   c { | α | = 1 , 2 Ω | E α | p α p α 1   1 + | u n | ( λ + θ ) q | u n | k + σ 1   d x       + Ω 1 + | u n | θ ( q 1 ) δ | u n | k + σ 1 δ   d x + Ω | f | | u n | k + σ   d x }  
(note that ( q 1 ) δ > q + δ ).
Taking into account (21) and the inequality
1 + | u n | 2 k + | u n | k +   if   k 1 ,
from (25), we obtain
1 2 θ ( q 1 ) | α | = 1 , 2 Ω | D α u n | p α | u n | k + σ 1   d x   c { | α | = 1 , 2 Ω | E α | p α   | u n | k + σ 1 + ( λ + θ ) q   d x + Ω | u n | k + σ 1 δ + θ ( q 1 ) δ   d x + Ω | f | | u n | k + σ + θ ( q 1 )   d x + | α | = 1 , 2 k ( λ + θ ) q Ω | E α | p α   | u n | k + σ 1   d x + k θ ( q 1 ) δ Ω | u n | k + σ 1 δ   d x + k θ ( q 1 ) Ω | f | | u n | k + σ   d x } ,  
for any k 1 .
By Sobolev’s embedding theorem and the above inequality, we obtain
[ Ω | | u n | k + σ 1 q + 1 | q *   d x ] q q *   c { | α | = 1 , 2 Ω | E α | p α   | u n | k + σ 1 + ( λ + θ ) q   d x + Ω | u n | k + σ 1 δ + θ ( q 1 ) δ   d x + Ω | f | | u n | k + σ + θ ( q 1 )   d x   + | α | = 1 , 2 k ( λ + θ ) q Ω | E α | p α   | u n | k + σ 1   d x + k θ ( q 1 ) δ Ω | u n | k + σ 1 δ   d x + k θ ( q 1 ) Ω | f | | u n | k + σ   d x }
for every k 1 and σ > 1 + q (note that if θ and λ verify condition (12), then 1 + q > 1 + ( λ + θ ) q and 1 + q > 1 + δ + θ ( q 1 ) δ ).
We denote by A n ( k ) the level set of | u n | , that is,
A n ( k ) = x Ω   :   | u n ( x ) | > k
and we denote by | A n ( k ) | the N-dimensional Lebesgue measure of A n ( k ) .
Let γ = σ 1 + q q * q . Applying Hölder’s inequality to (27) and taking into account assumptions (8), (9) and (12), we obtain
Ω | u n | k + γ   d x q q *   c { | α | = 1 , 2 E α r α p α   Ω | u n | k + γ   d x σ 1 + ( λ + θ ) q γ · | A n ( k ) | 1 p α r α σ 1 + ( λ + θ ) q γ + Ω | u n | k + γ   d x σ 1 δ + θ ( q 1 ) δ γ · | A n ( k ) | 1 σ 1 δ + θ ( q 1 ) δ γ   + f t Ω | u n | k + γ   d x σ + θ ( q 1 ) γ · | A n ( k ) | 1 1 t σ + θ ( q 1 ) γ + k ( λ + θ ) q | α | = 1 , 2 E α r α p α   Ω | u n | k + γ   d x σ 1 γ · | A n ( k ) | 1 p α r α σ 1 γ + k θ ( q 1 ) δ Ω | u n | k + γ   d x σ 1 δ γ · | A n ( k ) | 1 σ 1 δ γ   + k θ ( q 1 ) f t Ω | u n | k + γ   d x σ γ · | A n ( k ) | 1 1 t σ γ } .
Now, we set
φ ( u n ) = Ω | u n | k + γ   d x
and
χ = q q * ,   β 1 = σ 1 + ( λ + θ ) q γ ,   β 2 = σ 1 δ + θ ( q 1 ) δ γ ,   β 3 = σ + θ ( q 1 ) γ , β 4 = σ 1 γ ,   β 5 = σ 1 δ γ ,   β 6 = σ γ .
Then, inequality (28) becomes
        φ ( u n ) χ c { φ ( u n ) β 1 | A n ( k ) | 1 p α r α σ 1 + ( λ + θ ) q γ               + φ ( u n ) β 2 | A n ( k ) | 1 σ 1 δ + θ ( q 1 ) δ γ + φ ( u n ) β 3 | A n ( k ) | 1 1 t σ + θ ( q 1 ) γ + k ( λ + θ ) q φ ( u n ) β 4 | A n ( k ) | 1 p α r α σ 1 γ + k θ ( q 1 ) δ φ ( u n ) β 5 | A n ( k ) | 1 σ 1 δ γ + k θ ( q 1 ) φ ( u n ) β 6 | A n ( k ) | 1 1 t σ γ } .
Thanks to assumption (12), the exponents β 1 β 6 are less than χ . Therefore, we can apply Lemma 2 to the previous inequality, with
a 1 =   | A n ( k ) | 1 p α r α σ 1 + ( λ + θ ) q γ ,   a 2 = | A n ( k ) | 1 σ 1 δ + θ ( q 1 ) δ γ , a 3 =   | A n ( k ) | 1 1 t σ + θ ( q 1 ) γ ,   a 4 = k ( λ + θ ) q | A n ( k ) | 1 p α r α σ 1 γ , a 5 = k θ ( q 1 ) δ | A n ( k ) | 1 σ 1 δ γ ,   a 6 = k θ ( q 1 ) | A n ( k ) | 1 1 t σ γ ,
and we obtain
Ω | u n | k + γ   d x c i = 1 6 k τ i γ   | A n ( k ) | γ i ,
where
γ 1 = γ 1 ( λ + θ ) 1 p α r α σ 1 + ( λ + θ ) q γ , γ 2 = γ q + δ θ ( q 1 ) δ 1 σ 1 δ + θ ( q 1 ) δ γ γ 3 = γ ( q 1 ) ( 1 θ ) 1 1 t σ + θ ( q 1 ) γ , γ 4 = γ q 1 p α r α σ 1 γ γ 5 = γ q + δ 1 σ 1 δ γ γ 6 = γ q 1 1 1 t σ γ
and
  τ 1 = 0 , τ 2 = 0 , τ 3 = 0 ,   τ 4 = ( λ + θ ) , τ 5 = θ ( q 1 ) δ q + δ , τ 6 = θ .
Under assumptions of 0 θ < q p p ( q 1 ) and λ + θ < 1 , every number τ i , i = 1 , , 6 , is less than 1; furthermore, hypotheses (8), (9) and (12) ensure that it is possible to choose a large enough σ such that γ i > 1 for any i = 1 , , 6 .
Now, for every h > k 1 , with | u n | k + h k on A n ( h ) , from (30), we have
| A n ( h ) | i = 1 6 c   k τ i γ ( h k ) γ | A n ( k ) | γ i .
Hence, there exists i, i = 1 , , 6 , such that
1 6 | A n ( h ) | c   k τ i γ ( h k ) γ | A n ( k ) | γ i .
Therefore, using Lemma 3, we conclude that there exist two positive constants k * and d 0 (independent of n) such that
| A n ( k ) | = 0   for   every   k k * + d 0 .
Hence,
u n L ( Ω ) M   for   every   n N
with M = k * + d 0 , and the proof of the lemma is complete. □
The next lemma deals with the boundedness of u n in the energy space W ˚ 2 , p 1 , q ( Ω ) .
Lemma 6. 
Let hypotheses (5)–(9) be satisfied. Then, there exists a positive constant C, depending only on θ, N, q, p, ν 1 , ν 2 , | Ω | , E α L r α ( Ω ) , | α | = 1 , 2 , and | | f | | L t ( Ω ) , such that
| | u n | | W ˚ 2 , p 1 , q ( Ω ) C   f o r   e v e r y   n N .
Proof. 
Using v = u n as a test function in the integral identity (15) and applying the ellipticity condition (5), the growth condition (6) and Young’s inequality, we have
ν 1 | α | = 1 , 2 Ω | D α u n | p α ( 1 + | T n ( u n ) | ) θ ( p α 1 )   d x   τ | α | = 1 , 2 Ω | D α u n | p α ( 1 + | T n ( u n ) | ) θ ( p α 1 )   d x + C ( τ ) | α | = 1 , 2 Ω | E α | p α ( 1 + | u n | ) λ q + θ   d x     + Ω | f |   | u n |   d x .
Therefore, choosing a suitable 0 < τ < ν 1 and taking into account (31), from the above inequality, we obtain
Ω | α | = 1 , 2 | D α u n | p α   d x c | α | = 1 , 2 ( M + 1 ) ( λ + θ ) q + 1 Ω | E α | p α   d x + Ω | f |   d x .
and the lemma follows. □

4. Existence of Bounded Solution

From Lemma 5 and Lemma 6, we infer that there exists a subsequence of { u n } , not relabeled, and a function u W ˚ 2 , p 1 , q ( Ω ) L ( Ω ) such that
(a)
u n converges to u weakly in W ˚ 2 , p 1 , q ( Ω ) and almost everywhere in Ω;
(b)
u n converges to u weakly * in L ( Ω ) ;
(c)
u n converges to u strongly in W 1 , p ( Ω ) ;
(d)
u n converges to u strongly in L q ( Ω ) .
To pass to the limit in the approximating problems (15), first, we need to prove that the sequences D α u n , | α | = 1 , 2 , are convergent almost everywhere in Ω .
To this aim, we exploit the following compactness result, whose proof is in [13].
Lemma 7. 
Assume that hypotheses (5)–(7) hold and let z n be a sequence of functions such that
z n z   in   W ˚ 2 , p 1 , q ( Ω )   weakly   and ,   i . e . ,   in   Ω
and
lim n + | α | = 1 , 2 Ω [ A α ( x , z n , D 1 z n , D 2 z n )     A α ( x , z , D 1 z , D 2 z ) ] D α [ z n z ]   d x = 0 .  
Then, z n is relatively compact in the strong topology of W ˚ 2 , p 1 , q ( Ω ) .
We take v = u n u as a test function in the weak formulation of problem (15), and we obtain
| α | = 1 , 2 Ω A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) D α [ u n u ]   d x = | α | = 1 , 2 Ω E α u n 1 n + | u n |   | u n | λ ( p α 1 ) 1 + 1 n | u n | λ ( p α 1 ) D α [ u n u ]   d x + Ω f n [ u n u ]   d x .
Using (31), from the above equality, it follows that
| α | = 1 , 2 Ω A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) D α [ u n u ]   d x   ( 1 + M ) λ ( q 1 ) | α | = 1 , 2 Ω E α   D α [ u n u ]   d x + Ω f   [ u n u ]   d x
and therefore,
| α | = 1 , 2 Ω A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) A α ( x , u , D 1 u , D 2 u ) D α [ u n u ]   d x         ( 1 + M ) λ ( q 1 ) | α | = 1 , 2 Ω E α   D α [ u n u ]   d x + | α | = 1 , 2 Ω A α ( x , u , D 1 u , D 2 u )   D α [ u n u ]   d x + Ω f   [ u n u ]   d x  
The sums on the right-hand side of (36) tend to zero as n tends to + since u n converges to u weakly in W ˚ 2 , p 1 , q ( Ω ) , and A α ( x , u , D 1 u , D 2 u ) and E α belong to L p α ( Ω ) , | α | = 1 , 2 , thanks to (6) and (8). The last integral converges to zero as n tends to + because u n converges to u weakly * in L ( Ω ) .
On the other hand, the boundedness of u n L implies T n ( u n ) = u n for sufficiently large n; therefore, the hypotheses of Lemma 7 are satisfied, and we conclude that, up to a subsequence,
u n u   strongly   in   W ˚ 2 , p 1 , q ( Ω ) .
Proof of Theorem 1. 
Let v W ˚ 2 , p 1 , q ( Ω ) be a test function in (15).
Taking into account that T n ( u n ) = u n for n > M and using the growth condition (6) and the strong convergence of u n to u in W ˚ 2 , p 1 , q ( Ω ) , we have
lim n + | α | = 1 , 2 Ω A α ( x , T n ( u n ) , D 1 u n , D 2 u n ) D α v   d x = | α | = 1 , 2 Ω A α ( x , u , D 1 u , D 2 u ) D α v   d x .
Now, we define the sequence { Y n α } , where
Y n α ( x ) = E α ( x ) u n ( x ) 1 n + | u n ( x ) |   | u n ( x ) | λ ( q 1 ) 1 + 1 n | u n ( x ) | λ ( q 1 ) : Ω R N ,   if   | α | = 1 ,
and
Y n α ( x ) = E α ( x ) u n ( x ) 1 n + | u n ( x ) |   | u n ( x ) | λ ( p 1 ) 1 + 1 n | u n ( x ) | λ ( p 1 ) : Ω R N 2 ,   if   | α | = 2 .
Thanks to the convergence of u n ( x ) to u ( x ) , i.e., x Ω , the sequence Y n α ( x ) converges to E α ( x )   | u ( x ) | λ ( p α 1 ) 1   u ( x ) , | α | = 1 , 2 i.e., x Ω .
Furthermore, by exploiting (31), we deduce that
| E α ( x ) u n ( x ) 1 n + | u n ( x ) |   | u n ( x ) | λ ( p α 1 ) 1 + 1 n | u n ( x ) | λ ( p α 1 ) | M λ ( p α 1 )   | E α ( x ) | ,   | α | = 1 , 2
for any x Ω . Hence, by the Lebesgue Theorem,
Y n α E α   | u | λ ( p α 1 ) 1   u   strongly   in   L p α ( Ω ) ,   | α | = 1 , 2 .
We can pass to the limit as n + in the weak formulation (15), and we find that u is a weak solution of problem (10), in the sense of Definition 1.
Finally, the almost-everywhere convergence of { u n ( x ) } to u ( x ) in Ω and (31) yield the estimate
u L ( Ω ) M .
This completes the proof of Theorem 1. □

5. Proof of Theorem 2

We begin this section by recalling the following lemma according to Skripnik (see [29]). Let y R N be a fixed point. Given R > 0 , we denote by B R ( y ) an open ball centered on y with radius R.
Lemma 8. 
Let g W 1 , 1 ( B R ( y ) ) . Assume that there exists a measurable subset G B R ( y ) and two positive constants C and C such that
meas ( G ) C R N ,   max G | g | C .
Then, there exists a positive constant C, independent of R, such that
B R ( y ) | g |   d x C R B R ( y ) | β | = 1 | D β g |   d x + R N 1 .
Let Ω Ω be any strictly interior sub-region of Ω and d = dist Ω , Ω .
Let u W ˚ 2 , p 1 , q ( Ω ) L ( Ω ) be a weak solution of problem (10), such that
| u ( x ) | M   for   i . e . ,   x Ω .
We fix x 0 Ω , and for any R such that 0 < R < d 4 , we set
ω 1 ( R ) = ess   inf B R ( x 0 )   u ( x ) ,   ω 2 ( R ) = ess   sup B R ( x 0 )   u ( x ) ,   ω ( R ) = ω 2 ( R ) ω 1 ( R ) .
By virtue of Lemma 4.8 pag. 66 of [30], Theorem 2 will be proved as long as the inequality
ω ( R ) χ ω ( 2 R ) + R r
holds, where 0 < χ < 1 , depending only on known parameters and independent of R, and r is a positive number such that the following inequalities hold:
| α | p α + r ( q p α ) q ,   | α | = 1 ,   2 ,           r q + p q q 2 p q ,     r < min 1 N q t , q 2 p q p .
To prove (38), we fix 0 < R < min 1 , d 4 , and we consider the sets
G 1 ( R ) = x B R ( x 0 )   :   u ( x ) ω 1 ( R ) + ω 2 ( R ) 2 ,   G 2 ( R ) = B R ( x 0 ) G 1 ( R ) .
At least one of the following inequalities holds:
meas G 1 ( 2 R ) 1 2 meas B 2 R ( x 0 ) ,
or
meas G 2 ( 2 R ) 1 2 meas B 2 R ( x 0 ) .
If inequality (40) holds, we define the function v 0 : Ω R as follows:
v 0 ( x ) = 1 + log 2 ω ω 2 u ( x ) + R r if   x B 2 R ( x 0 ) 0 if   x Ω B 2 R ( x 0 ) ,
where ω = ω ( 2 R ) ,   ω 2 = ω 2 ( 2 R ) . Otherwise, if inequality (41) holds, the function v 0 is defined by
v 0 ( x ) = 1 + log 2 ω u ( x ) ω 1 + R r if   x B 2 R ( x 0 ) 0 if   x Ω B 2 R ( x 0 ) ,
where ω 1 = ω 1 ( 2 R ) .
For the sake of simplicity, we assume that (40) holds, so v 0 is the function defined in (42).
Our aim is to prove that
ess   sup B 2 R ( x 0 )   v 0 ( x ) M
with M depending on N, p, q, θ , | | u | | L ( Ω ) , | | f | | L t ( Ω ) and | | E α | | L r α ( Ω ) , with | α | = 1 , 2 and d .
As a matter of fact, if (43) holds, then u ( x ) ω 2 ( 2 R ) 2 e M ω ( 2 R ) + R r for i.e., x B 2 R ( x 0 ) ; therefore, ω ( R ) ( 1 2 e M ) ω ( 2 R ) + R r , which gives inequality (38) with χ = 1 2 e M .
We can assume that
ω ( 2 R ) e R r 2
which implies v 0 ( x ) 1 , i.e., in B 2 R ( x 0 ) ; otherwise, inequality (38) holds.
We fix a function ψ 0 C 0 ( R ) such that
  0 ψ 0 ( s ) 1   for   every   s R ,   ψ 0 ( s ) = 1   if   | s | 1 ,   ψ 0 ( s ) = 0   if   | s | 2 .
For any x Ω , we set ψ ( x ) = ψ 0 | x x 0 | R and
v ( x ) = [ v 0 ( x ) ] k ( ω 2 u + R r ) q 1 ψ s ( x )
with k 0 , s q . Simple calculations show that v W ˚ 2 , p 1 , q ( Ω ) L ( Ω ) , and the following assertion holds:
D α v = k   [ v 0 ] k 1 ( ω 2 u + R r ) q D α u ψ s + ( q 1 )   [ v 0 ] k ( ω 2 u + R r ) q D α u ψ s + R | α | ( u )
where, for i.e., x Ω ,
| R | α | ( u ) | c s   [ v 0 ] k ψ s 1 ( ω 2 u + R r ) q 1   1 R   if   | α | = 1 | R | α | ( u ) | c   ( k + s + 1 ) 2   [ v 0 ] k ψ s 2 ( ω 2 u + R r ) q 1 1 R 2 + | β | = 1 | D β u | 2   ψ 2 ( ω 2 u + R r ) 2   if   | α | = 2
Now, we test the integral identity (11) with v. By using (5), (6) and (37), we obtain
( q 1 ) ( 1 + M ) θ ( q 1 ) Ω [ v 0 ] k ( ω 2 u + R r ) q | α | = 1 , 2 | D α u | p α ψ s   d x   c ( k + 1 ) J 1 + J 2 + J 3 + Ω | f |   [ v 0 ] k ( ω 2 u + R r ) q 1 ψ s   d x
where
J 1 = | α | = 1 , 2 Ω | E α |   | u | λ ( p α 1 ) [ v 0 ] k | D α u | ( ω 2 u + R r ) q ψ s   d x ,
J 2 = | α | = 1 , 2 Ω | E α |   | u | λ ( p α 1 ) | R | α | ( u ) |   d x ,
and
J 3 = | α | = 1 , 2 Ω | A α ( x , D 1 u , D 2 u ) |   | R | α | ( u ) |   d x .
Let us estimate J 1 . By using Young’s inequality with ε > 0 and taking into account (37), we derive
J 1 ε Ω [ v 0 ] k ( ω 2 u + R r ) q | α | = 1 , 2 | D α u | p α ψ s   d x   + C ( c , ε ) ( M + 1 ) q | α | = 1 , 2 Ω [ v 0 ] k   | E α | p α p α 1 ( ω 2 u + R r ) q ψ s   d x .
In order to estimate J 2 , we use the inequalities in (47). We obtain
J 2 c | α | = 1 , 2 Ω | E α |   | u | λ ( p α 1 ) ( k + s + 1 ) | α |   [ v 0 ] k ( ω 2 u + R r ) q 1   1 R | α |   ψ s | α |   d x + | α | = 2 Ω | E α |   | u | λ ( p 1 ) ( k + s + 1 ) 2 [ v 0 ] k ( ω 2 u + R r ) q + 1   | β | = 1 | D β u | 2   ψ s   d x .  
Since | α | p α + r ( q p α ) q , by using Young’s inequality and (37), the first sum on the right-hand side can be evaluated as follows:
| α | = 1 , 2 Ω | E α |   | u | p α 1 ( k + s + 1 ) | α |   [ v 0 ] k ( ω 2 u + R r ) q 1   1 R | α |   ψ s | α |   d x   c ( M + k + s + 1 ) q | α | = 1 , 2 Ω [ v 0 ] k   | E α | p α p α 1 ( ω 2 u + R r ) q ψ s   d x + Ω [ v 0 ] k   ψ s | α | p α R q   d x .
Using the assumption r q + p q q 2 p q and, again, Young’s inequality and (37), the last sum on the right-hand side in (53) can be estimated as
| α | = 2 Ω | E α |   | u | λ ( p 1 ) ( k + s + 1 ) 2 [ v 0 ] k ( ω 2 u + R r ) q + 1   | β | = 1 | D β u | 2   ψ s   d x   ε Ω [ v 0 ] k ( ω 2 u + R r ) q | α | = 1 | D α u | q ψ s   d x + C ( c , ε ) ( M + k + s + 1 ) q | α | = 2 Ω [ v 0 ] k   | E α | p p 1 ( ω 2 u + R r ) q   ψ s   d x + | α | = 2 Ω [ v 0 ] k   ψ s R q   d x .
From inequalities (53)–(55), we obtain
J 2 ε Ω | α | = 1 | D α u | q [ v 0 ] k ( ω 2 u + R r ) q ψ s   d x + C ( c , ε ) ( M + k + s + 1 ) q | α | = 1 , 2 Ω [ v 0 ] k   | E α | p α p α 1 ( ω 2 u + R r ) q ψ s   d x + Ω [ v 0 ] k   ψ s q R q   d x .
Finally, let us estimate J 3 . By using (6) and taking into account (47), we have
J 3 c { | α | = 1 , 2 Ω | α | = 1 , 2 | D α u | p α p α 1 p α ( k + s + 1 ) | α |   [ v 0 ] k R | α |   ( ω 2 u + R r ) q 1 ψ s | α |   d x + Ω | α | = 1 , 2 | D α u | p α p 1 p ( k + s + 1 ) 2 [ v 0 ] k ( ω 2 u + R r ) q + 1 | β | = 1 | D β u | 2 ψ s   d x } .  
Applying Young’s inequality with the exponents p α p α 1 and p α , we can evaluate the first integrals in (57) as follows:
| α | = 1 , 2 Ω | α | = 1 , 2 | D α u | p α p α 1 p α ( k + s + 1 ) | α |   [ v 0 ] k   ψ s | α | R | α |   ( ω 2 u + R r ) q 1   d x       ε Ω | α | = 1 , 2 | D α u | p α [ v 0 ] k   ψ s ( ω 2 u + R r ) q   d x + C ( c , ε ) ( k + s + 1 ) q Ω [ v 0 ] k   ψ s q R q   d x ,
where we have used condition (39), that is, | α | p α + r ( q p α ) q , | α | = 1 , 2 .
In the last integrals of (57), we use Young’s inequality with the exponents p p 1 , q 2 and p q q 2 p and condition (39): r q + p q q 2 p q . We obtain
Ω | α | = 1 , 2 | D α u | p α p 1 p ( k + s + 1 ) 2 [ v 0 ] k ( ω 2 u + R r ) q + 1 | β | = 1 | D α u | 2 ψ s   d x   ε Ω | α | = 1 , 2 | D α u | p α [ v 0 ] k   ψ s ( ω 2 u + R r ) q   d x + C ( c , ε ) ( k + s + 1 ) q Ω [ v 0 ] k   ψ s R q   d x .
From (58) and (59), we deduce
J 3 ε Ω | α | = 1 , 2 | D α u | p α [ v 0 ] k   ψ s ( ω 2 u + R r ) q   d x + C ( c , ε ) ( k + s + 1 ) q Ω [ v 0 ] k   ψ s R q   d x .  
Finally, we estimate the integral involving the datum. Since (37) holds, we have
Ω | f |   [ v 0 ] k ( ω 2 u + R r ) q 1 ψ s   d x c ( 2 M + 1 ) Ω | f |   [ v 0 ] k ( ω 2 u + R r ) q ψ s   d x .
Now, gathering (48), (52), (56), (60) and (61) and choosing a suitable ε > 0 , we obtain
Ω | α | = 1 , 2 | D α u | p α [ v 0 ] k   ψ s ( ω 2 u + R r ) q   d x   c ( 1 + k + s ) q ( M + 1 ) q + θ ( q 1 ) Ω F   [ v 0 ] k   ψ s ( ω 2 u + R r ) q   d x + Ω [ v 0 ] k   ψ s q R q   d x
where we have denoted by F the following function:
F = | α | = 1 , 2 | E α | p α p α 1 + | f | + 1 .
Thanks to (8) and (9), it follows that there exists τ > N q such that F L τ ( Ω ) . Therefore, choosing r < 1 N q τ and applying Hölder’s inequality, from (62), we obtain
Ω | α | = 1 , 2 | D α u | p α [ v 0 ] k   ψ s ( ω 2 u + R r ) q   d x   c ( 1 + k + s ) q { 1 R r q   Ω | F | τ   d x 1 τ Ω | [ v 0 ] k   ψ s q | τ τ 1   d x τ 1 τ + 1 R q N τ Ω | [ v 0 ] k   ψ s q | τ τ 1   d x τ 1 τ }     c ( 1 + k + s ) q 1 R q N τ Ω | [ v 0 ] k   ψ s q | τ τ 1   d x τ 1 τ
The above relation is crucial for organizing the iterative Moser’s method.
Given k 0 and s > 0 , let us define
J ( k , s ) = 1 R N   Ω [ v 0 ] k ψ s   d x .
The following Lemma holds:
Lemma 9. 
We assume that conditions (5)–(9) are satisfied. Let u W ˚ 2 , p 1 , q ( Ω ) be a bounded solution of problem (10).
Then, if k > 0 and 2 q * < s < C 0 ( k + 1 ) ( C 0 is an absolute constant that we shall define later), the inequality
J ( k , s ) c ( k + 1 ) q * J ( k l , s l 2 l q * ) 1 l
holds, where
l = τ τ 1   N q N < 1 .
Proof. 
Let k > 0 and 2 q * < s < C 0 ( k + 1 ) . Applying Sobolev’s embedding to the function [ v 0 ] k q *   ψ s q * and taking into account that v 0 ( x ) 1 , we obtain
J ( k , s ) c   S 1 ( k + s + 1 ) q * R N ( Ω | β | = 1 | D β u | q [ v 0 ] k q q *   ψ s q q * q ( ω 2 u + R r ) q   d x + 1 R q Ω [ v 0 ] k q q *   ψ s q q * q   d x ) q * q ,
where S 1 is the Sobolev constant.
Now, estimating the first addend on the right-hand side of the above inequality by means of (64) with k q q * and s q q * q instead of k and s and the second one by means of Hölder’s inequality, we obtain
J ( k , s ) c   C 0 ( 1 + k ) q * 1 R N Ω [ v 0 ] k k q q * τ τ 1   ψ ( s q q * q ) τ τ 1   d x τ 1 τ q * q
and (65) follows. □
For i = 0 , 1 , 2 , , and C 0 such that C 0 > 2 l 1 l q * q , we define
k i = q l i ,   s i = 2 l q * 1 l ( l i 1 ) ,   J i = J ( k i , s i )
In the next lemma, we will prove the boundedness of J 0 = J ( q , 0 ) .
Lemma 10. 
We assume that conditions (5)–(9) are satisfied. Let u W ˚ 2 , p 1 , q ( Ω ) be a bounded solution of problem (10). Then, the inequality
B 2 R ( x 0 ) [ v 0 ] q   d x C 1 R N
holds, where C 1 is a positive constant depending only on known parameters and independent of R.
Proof. 
We note that 1 [ v 0 ( x ) ] q ( 1 + log 4 ) q for any x G 1 ( R ) , so we can apply Lemma 8 to the function [ v 0 ] q W 1 , 1 B 2 R ( x 0 ) and G = G 1 ( R ) .
By means of Young’s inequality with ε > 0 , we obtain
1 R N B 2 R ( x 0 ) [ v 0 ] q   d x 1 + q R N 1 B 2 R ( x 0 ) [ v 0 ] q 1 ω 2 u + R r | α | = 1 | D α u |   d x   c { 1 + R N ε B 2 R ( x 0 ) [ v 0 ] q   d x + C ( ε ) R N q B 2 R ( x 0 ) 1 ( ω 2 u + R r ) q | α | = 1 | D α u | q   d x } .
Now, we estimate the last integral in the above inequality.
We then consider the following cut-off function:
φ ( x ) = ψ 0 x x 0 2 R ,   x Ω
where ψ 0 is the same function defined in (45), and we consider the following test function:
v 1 ( x ) = 1 ( ω 2 u ( x ) + R r ) q 1 φ q ( x ) .
Substituting v 1 into the integral identity (11) and proceeding in the same way as we obtained (64), we deduce
B 2 R ( x 0 ) | α | = 1 , 2 | D α u | p α 1 ( ω 2 u + R r ) q   d x c R q N τ meas B 4 R ( x 0 ) τ 1 τ c   R N q
Choosing a suitable 0 < ε < 1 and taking into account (70), from (69), we obtain
1 R N B 2 R ( x 0 ) [ v 0 ] q   d x c
and the lemma is proved. □
From Lemmas 9 and 10, we deduce
J i 1 k i c J 0 1 q   for   i = 0 , 1 , 2 ,
and
v 0 L B R ( x 0 ) = lim i + 1 R N B R ( x 0 ) [ v 0 ] k i   d x 1 k i c lim sup i + J i 1 k i c   J 0 1 q .
Therefore, (43) holds, and the proof of Theorem 2 is now complete.

Funding

This research received no external funding.

Data Availability Statement

The original contributions presented in this study are included in the article. Further inquiries can be directed to the corresponding author.

Acknowledgments

The author thanks the anonymous reviewers for helpful comments that improved the original manuscript. The author thanks G. Rita Cirmi and S. Leonardi for their useful discussions and suggestions. This study has been supported by Project EEEP&DLaD–Piano della Ricerca di Ateneo 2020–2022–PIACERI and by Piano della Ricerca 2024–2026 EdP.EReMo—”Equazioni differenziali alle derivate parziali: esistenza, regolarità e molteplicità delle soluzioni”. The author is a member of the Gruppo Nazionale per l’Analisi Matematica, la Probabilità e le loro Applicazioni (GNAMPA) of the Istituto Nazionale di Alta Matematica (INdAM).

Conflicts of Interest

The author declares no conflicts of interest.

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D’Asero, S. Existence of Bounded Solutions for a Class of Degenerate Fourth-Order Elliptic Equations with Convection Terms. Mathematics 2025, 13, 3. https://doi.org/10.3390/math13010003

AMA Style

D’Asero S. Existence of Bounded Solutions for a Class of Degenerate Fourth-Order Elliptic Equations with Convection Terms. Mathematics. 2025; 13(1):3. https://doi.org/10.3390/math13010003

Chicago/Turabian Style

D’Asero, Salvatore. 2025. "Existence of Bounded Solutions for a Class of Degenerate Fourth-Order Elliptic Equations with Convection Terms" Mathematics 13, no. 1: 3. https://doi.org/10.3390/math13010003

APA Style

D’Asero, S. (2025). Existence of Bounded Solutions for a Class of Degenerate Fourth-Order Elliptic Equations with Convection Terms. Mathematics, 13(1), 3. https://doi.org/10.3390/math13010003

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